A theoretical investigation of the possible detection of C24 in space

Bibcode
2020FNCN...28..637S
DOI
10.1080/1536383X.2020.1731735
Sadjadi, SeyedAbdolreza; Kwok, Sun; Cataldo, Franco; García-Hernández, D. A.; Manchado, Arturo
Referencia bibliográfica

Fullerene Nanotubes and Carbon Nanostructures

Fecha de publicación:
8
2020
Número de autores
5
Número de autores del IAC
2
Número de citas
4
Número de citas referidas
4
Descripción
Astronomical infrared spectral features at ~6.6, 9.8 and 20 micronm have recently been suggested as being due to the planar graphene form of C24 carbon cluster. Here we report density functional theory and coupled cluster calculations on wavefunctions stability, relative energies, and infrared spectra of four different types of C24 isomers, including the graphene and fullerene forms. The types of vibrational motions under these bands are also discussed. Among the four isomers, we find that the astronomical data are best approximated by the graphene form of C24.
Proyectos relacionados
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Nucleosíntesis y procesos moleculares en los últimos estados de la evolución estelar

Las estrellas de masa baja e intermedia (M < 8 masas solares, Ms) representan la mayoría de estrellas en el Cosmos y terminan sus vidas en la Rama Asintótica de las Gigantes (AGB) - justo antes de formar Nebulosas Planetarias (NPs) - cuando experimentan procesos nucleosintéticos y moleculares complejos. Las estrellas AGB son importantes

Domingo Aníbal
García Hernández
En ejecución
Tipo
Con árbitro
Sistema Solar y Sistemas Planetarios (SEYSS)
Física estelar e interestelar (FEEI)
La Vía Láctea y el Grupo Local (MWLG)

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